CWWDL 8594

0.02 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.0

C_lit

0.72

C_dup

C3 classification DC

Number of members (P>50%) 18

Radius (P>50% members) 8.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.72 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 8594 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 8594 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	88.035	29.76	0.24	0.1	-1.598	59.283
Chi et al.	2023	87.939	29.681	0.262	0.12	-1.583	32.366

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Chi et al.	2023	–	–	–	214	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Koposov 43	28.0	88.08	29.9	0.19	-0.08	-1.67	12.03	0.9

💡 Note: The % column shows the percentage of members that CWWDL 8594 shares with each listed object.

Visualization

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